コード例 #1
0
ファイル: infotheo.py プロジェクト: ChadFulton/statsmodels
def discretize(X, method="ef", nbins=None):
    """
    Discretize `X`

    Parameters
    ----------
    bins : int, optional
        Number of bins.  Default is floor(sqrt(N))
    method : string
        "ef" is equal-frequency binning
        "ew" is equal-width binning

    Examples
    --------
    """
    nobs = len(X)
    if nbins == None:
        nbins = np.floor(np.sqrt(nobs))
    if method == "ef":
        discrete = np.ceil(nbins * stats.rankdata(X)/nobs)
    if method == "ew":
        width = np.max(X) - np.min(X)
        width = np.floor(width/nbins)
        svec, ivec = stats.fastsort(X)
        discrete = np.zeros(nobs)
        binnum = 1
        base = svec[0]
        discrete[ivec[0]] = binnum
        for i in range(1,nobs):
            if svec[i] < base + width:
                discrete[ivec[i]] = binnum
            else:
                base = svec[i]
                binnum += 1
                discrete[ivec[i]] = binnum
    return discrete
コード例 #2
0
def discretize(X, method="ef", nbins=None):
    """
    Discretize `X`

    Parameters
    ----------
    bins : int, optional
        Number of bins.  Default is floor(sqrt(N))
    method : string
        "ef" is equal-frequency binning
        "ew" is equal-width binning

    Examples
    --------
    """
    nobs = len(X)
    if nbins is None:
        nbins = np.floor(np.sqrt(nobs))
    if method == "ef":
        discrete = np.ceil(nbins * stats.rankdata(X)/nobs)
    if method == "ew":
        width = np.max(X) - np.min(X)
        width = np.floor(width/nbins)
        svec, ivec = stats.fastsort(X)
        discrete = np.zeros(nobs)
        binnum = 1
        base = svec[0]
        discrete[ivec[0]] = binnum
        for i in range(1,nobs):
            if svec[i] < base + width:
                discrete[ivec[i]] = binnum
            else:
                base = svec[i]
                binnum += 1
                discrete[ivec[i]] = binnum
    return discrete
コード例 #3
0
ファイル: foldspectra.py プロジェクト: ezietsman/msc-thesis
    print phasetemp
    phase.append(phasetemp)
print '...Done!\n'

head = pf.getheader(ff[0])
start = head['CRVAL1']
step = head['CDELT1']
length = head['NAXIS1']
x = start + pl.arange(0,length)*step
hi = x > 6500
low = x < 6625
xx = hi*low


# now get the phases, sort them and find the order of numbers.
phase,argsort = stats.fastsort(pl.array(phase))



im = pl.array([pf.getdata(ff[i])[xx]-pl.median(pf.getdata(ff[i])[xx]) for i in argsort])

print im
#im = pl.array([allspec[i].count for i in range(len(allspec))])

# phases are not equispaced, need to interpolate im on to regular phase grid.

#l,w = pl.shape(im)

#x = pl.linspace(0.0,1.0,l)
#im2 = 1.0*pl.zeros((l,w))
コード例 #4
0
# start with lpDNO @ 829 c/d. check if this is the actual frequency
# calculate phase for every spectrum and assign number to it
#period = 1.0/3627.965
#t0 = float(pf.getheader(ff[0])['HJD'])

print 'Calculating phase...\n'
for i in range(len(ff[:-2])):
    temp = ((float(pf.getheader(ff[i])['HJD']) - T0)/P)
    phase.append(temp)
print '...Done!\n'


# now get the phases, sort them and find the order of numbers.
phase = pl.array(phase)
phase2 = (pl.array(phase) - phase[0]) / P2
phase2,argsort = stats.fastsort(pl.array(phase2))


# speed of light in km/s
c = 2.99792458e5
v = 1500.0
for i in ff:
    
    
    # subtract average from spectrum
    data = pf.getdata(i)# - ave
    head = pf.getheader(i)
    
    
    # write average subtracted spectrum to new fits file
    #pf.writeto('avesub%s'%i,data=data,header=head)
コード例 #5
0
ファイル: Spec_vs_phot.py プロジェクト: ezietsman/msc-thesis
pl.subplot(221)
pl.plot(pl.array(t-int(t[0])),pl.array(big))
ylo,yhi = pl.ylim()
pl.ylim(yhi,ylo)
#pl.xlim(0.3,0.6)
pl.title('Spectrum lightcurve')
pl.xlabel('HJD')
pl.ylabel('Total spectrum Mag')

pl.subplot(222)
f,a = ast.signal.dft(t,big,3000,3934,0.1)
pl.title('Spectrum periodogram')
pl.xlabel('Frequency [Cycles/Day]')
pl.ylabel('Amplitude [mag]')
pl.plot(f,a,'g-')
sorted,argsort = sci.fastsort(a)
print 'Max amplitude of %s at %s cycles/day' % (sorted[-1],f[argsort[-1]])
pl.subplot(223)
pl.plot(x,y,'.')
pl.title('Photometry lightcurve')
ylo,yhi = pl.ylim()
pl.ylim(yhi,ylo)
pl.xlabel('HJD')
pl.ylabel('Relative Magnitude')

pl.subplot(224)
f,a = ast.signal.dft(x,y,0,3934,0.1)
pl.title('Photometry periodogram')
pl.xlabel('Frequency [Cycles/Day]')
pl.ylabel('Amplitude [mag]')
pl.plot(f,a,'g-')
コード例 #6
0
temp.append(date)
temp.append(phase)
temp.append(flux)

pl.save('HeIIlightcurve.dat',pl.array(temp).transpose())

lt = phase < 7.9

date = date[lt]
flux = pl.array(flux)[lt]
phase = pl.array(phase)[lt]
# flatten lightcurve using fourier method
fft = sci.fft(flux)
fft[0:4] = 0.0
fft[-4:] = 0.0
flux = sci.ifft(fft)

f,a = ast.signal.dft(date,flux,0,4000,1)
pl.figure()
pl.subplot(211)
pl.plot(phase,flux)
#pl.ylim(-5e-8,5e-8)
pl.subplot(212)
pl.plot(f,a)
sort,argsort = stats.fastsort(a)
print 'Max amplitude of %s at %s' % (a[argsort[-1]],f[argsort[-1]])
#print 'Second highest amplitude of %s at %s' % (a[argsort[-2]],f[argsort[-2]])
pl.show()


コード例 #7
0
ファイル: FTstats2.py プロジェクト: ezietsman/msc-thesis
    cof = pl.polyfit(x_bins[i]-xave,y_bins[i],3)
    z_bins.append(pl.polyval(cof,x_bins[i]-xave))
    

f = string.split(raw_input('Start End freq  : '))
f0 = float(f[0])
f1 = float(f[1])

print f0,f1
# now do fourier transform on every bins and give stats
ft_bins = [ast.signal.dft(x_bins[i],y_bins[i]-z_bins[i],f0,f1,1) for i in range(n)]

#print pl.shape(ft_bins)
print '\nBin\t','Amp\t\t\t','F c/d\t\t','F(s)\n\n'
for i in range(n):
    sort, argsort = stats.fastsort(ft_bins[i][1])
    amp = ft_bins[i][1][argsort[-1]]
    freq = ft_bins[i][0][argsort[-1]]
    print i,'\t',amp,'\t',freq,'\t',86400.0/freq
print '\n\n\n'


# make plots
pl.figure(figsize=(9,12))
for i in range(n):
    plots = '%s1%s' % (n,i+1)
    pl.subplot(plots)
    pl.plot(ft_bins[i][0],ft_bins[i][1],'k')


pl.figure(figsize=(9,12))